http://solar.gmu.edu/heliophysics/api.php?action=feedcontributions&feedformat=atom&user=Abemporad
heliophysics - User contributions [en]
2026-08-10T21:58:24Z
User contributions
MediaWiki 1.31.0
http://solar.gmu.edu/heliophysics/index.php?title=List_of_CMEs_for_WG5_Analysis&diff=2389
List of CMEs for WG5 Analysis
2015-03-10T15:47:20Z
<p>Abemporad: </p>
<hr />
<div><div style="font-size: 150%;"><span style="color:red">'''List of near-Sun Observations/Determinations of CME Magnetic Fields for WG5'''</span></div><br />
<br />
{| class="wikitable"<br />
|-<br />
! Date and Time<br />
! Solar Source (AR # or location)<br />
! Method of Magnetic Field Determination<br />
! Publication<br />
! Miscellaneous<br />
! Submitter contact<br />
<br />
|- USER ENTRY ADD your inputs in blocks such as the following<br />
| 2011/06/07 06:47 UT<br />
| AR NOAA 11226 (CME propagating on the west limb)<br />
| The magnetic field in the corona is determined by applying the Rankine-Hugoniot equations to LASCO C2 and C3 white-light images of the CME-driven shock in order to derive a map of the shock Alfvenic Mach number<br />
| Bemporad, A. & Mancuso, S. 2010, ApJ 720, 130 (also Bemporad, A., Susino, R., & Mancso, S. ApJ, in preparation)<br />
| <br />
| R. Susino (susino@oato.inaf.it) and A. Bemporad (bemporad@oato.inaf.it)}</div>
Abemporad
http://solar.gmu.edu/heliophysics/index.php?title=List_of_CMEs_for_WG5_Analysis&diff=2388
List of CMEs for WG5 Analysis
2015-03-10T14:32:36Z
<p>Abemporad: </p>
<hr />
<div><div style="font-size: 150%;"><span style="color:red">'''List of near-Sun Observations/Determinations of CME Magnetic Fields for WG5'''</span></div><br />
<br />
{| class="wikitable"<br />
|-<br />
! Date and Time<br />
! Solar Source (AR # or location)<br />
! Method of Magnetic Field Determination<br />
! Publication<br />
! Miscellaneous<br />
! Submitter contact<br />
<br />
|- USER ENTRY ADD your inputs in blocks such as the following<br />
| 2011/06/07 06:47 UT<br />
| AR NOAA 11226 (CME propagating on the west limb)<br />
| The magnetic field strength in the corona is determined by applying the Rankine-Hugoniot equations to LASCO C2 and C3 white-light images of the CME-driven shock in order to derive a map of the shock Alfvenic Mach number<br />
| http://adsabs.harvard.edu/abs/2014cosp...40E.272B (ApJ in preparation)<br />
| <br />
| R. Susino (susino@oato.inaf.it) and A. Bemporad (bemporad@oato.inaf.it)}</div>
Abemporad
http://solar.gmu.edu/heliophysics/index.php?title=List_of_CMEs_for_WG5_Analysis&diff=2387
List of CMEs for WG5 Analysis
2015-03-10T13:14:33Z
<p>Abemporad: </p>
<hr />
<div><div style="font-size: 150%;"><span style="color:red">'''List of near-Sun Observations/Determinations of CME Magnetic Fields for WG5'''</span></div><br />
<br />
{| class="wikitable"<br />
|-<br />
! Date and Time<br />
! Solar Source (AR # or location)<br />
! Method of Magnetic Field Determination<br />
! Publication<br />
! Miscellaneous<br />
! Submitter contact<br />
<br />
|- USER ENTRY ADD your inputs in blocks such as the following<br />
|<br />
|<br />
|<br />
|<br />
|<br />
|<br />
|}</div>
Abemporad
http://solar.gmu.edu/heliophysics/index.php?title=List_of_CMEs_for_WG5_Analysis&diff=2386
List of CMEs for WG5 Analysis
2015-03-10T13:14:14Z
<p>Abemporad: </p>
<hr />
<div><div style="font-size: 150%;"><span style="color:red">'''List of near-Sun Observations/Determinations of CME Magnetic Fields for WG5'''</span></div><br />
<br />
{| class="wikitable"<br />
|-<br />
! Date and Time<br />
! Solar Source (AR # or location)<br />
! Method of Magnetic Field Determination<br />
! Publication<br />
! Miscellaneous<br />
! Submitter contact<br />
<br />
|- USER ENTRY ADD your inputs in blocks such as the following<br />
|Test<br />
|event<br />
|to<br />
|verify<br />
|table<br />
|works<br />
|}</div>
Abemporad
http://solar.gmu.edu/heliophysics/index.php?title=List_of_CMEs_for_WG5_Analysis&diff=2385
List of CMEs for WG5 Analysis
2015-03-10T13:12:08Z
<p>Abemporad: </p>
<hr />
<div><div style="font-size: 150%;"><span style="color:red">'''List of near-Sun Observations/Determinations of CME Magnetic Fields for WG5'''</span></div><br />
<br />
{| class="wikitable"<br />
|-<br />
! Date and Time<br />
! Solar Source (AR # or location)<br />
! Method of Magnetic Field Determination<br />
! Publication<br />
! Miscellaneous<br />
! Submitter contact<br />
<br />
|- USER ENTRY ADD your inputs in blocks such as the following<br />
|<br />
|<br />
|<br />
|<br />
|<br />
|<br />
|}</div>
Abemporad
http://solar.gmu.edu/heliophysics/index.php?title=List_of_CMEs_for_WG5_Analysis&diff=2384
List of CMEs for WG5 Analysis
2015-03-10T13:11:48Z
<p>Abemporad: </p>
<hr />
<div><div style="font-size: 150%;"><span style="color:red">'''List of near-Sun Observations/Determinations of CME Magnetic Fields for WG5'''</span></div><br />
<br />
{| class="wikitable"<br />
|-<br />
! Date and Time<br />
! Solar Source (AR # or location)<br />
! Method of Magnetic Field Determination<br />
! Publication<br />
! Miscellaneous<br />
! Submitter contact<br />
<br />
|- USER ENTRY ADD your inputs in blocks such as the following<br />
|<br />
|<br />
|<br />
|<br />
|<br />
|<br />
|}<br />
<br />
TEST EDIT</div>
Abemporad
http://solar.gmu.edu/heliophysics/index.php?title=The_ISEST_Event_List&diff=2383
The ISEST Event List
2015-03-04T07:56:36Z
<p>Abemporad: /* 2011 */</p>
<hr />
<div>This is a list of ICMEs arranged by year. The ICMEs are cataloged by the first appearence of a signature in-situ. To add an event that is not present in the list, follow the how to guide at [[Creating A New Event Page]]<br />
<br />
==2007==<br />
[[05/21/2007 21:00:00 UTC]] (ICME+CIR) <br \><br />
[[11/19/2007 17:00:00 UTC]] (published)<br \><br />
<br />
==2008==<br />
[[09/17/2008 04:20:00 UTC]] (published) <br \><br />
[[12/17/2008 03:30:00 UTC]] (published) <br \><br />
<br />
==2009==<br />
[[01/26/2009 05:00:00 UTC]] (ICME like, Kilpua et al. definition)<br \><br />
[[02/03/2009 22:00:00 UTC]] (ICME like)<br \><br />
[[08/30/2009 00:16:00 UTC]] (ICME, published)<br \><br />
[[09/30/2009 08:00:00 UTC]] (ICME like)<br \><br />
[[10/29/2009 12:30:00 UTC]] (ICME like)<br \><br />
[[11/14/2009 10:00:00 UTC]] (ICME like)<br \><br />
<br />
==2010==<br />
[[01/01/2010 22:00:00 UTC]] (ICME like) <br /><br />
[[04/05/2010 08:00:00 UTC]] (published) <br /><br />
[[04/12/2010 01:00:00 UTC]] (published) <br /><br />
[[05/28/2010 21:00:00 UTC]] (published) <br /><br />
[[06/21/2010 08:00:00 UTC]] (published) <br /><br />
[[08/03/2010 16:00:00 UTC]] (published) <br /><br />
[[12/28/2010 12:00:00 UTC]] (ICME like) <br /><br />
<br />
==2011==<br />
[[02/18/2011 00:00:00 UTC]] (published) <br /><br />
[[03/30/2011 01:00:00 UTC]] (long duration, over-expanding? ICME)<br /><br />
[[06/07/2011 06:26:00 UTC]] (ICME)<br \><br />
[[06/16/2011 03:00:00 UTC]] (ICME like)<br /><br />
[[07/03/2011 01:00:00 UTC]] (ICME like) <br /><br />
[[08/05/2011 18:00:00 UTC]] (published)<br /><br />
[[09/09/2011 11:46:00 UTC]] (ICME) <br /><br />
[[09/17/2011 15:00:00 UTC]] (ICME) <br /><br />
[[10/22/2011 22:00:00 UTC]] (ICME like)<br /><br />
[[10/24/2011 17:38:00 UTC]] (ICME)<br /><br />
[[11/01/2011 08:00:00 UTC]] (ICME like)<br /><br />
<br />
==2012==<br />
[[01/22/2012 05:00:00 UTC]] (published)<br /><br />
[[01/24/2012 14:36:00 UTC]] (ICME like) (published)<br /><br />
[[03/07/2012 03:28:00 UTC]] (ICME like)<br /><br />
[[03/08/2012 11:00:00 UTC]] (published)<br /><br />
[[03/12/2012 08:28:00 UTC]] <br /><br />
[[03/15/2012 13:00:00 UTC]] (ICME)<br /><br />
[[04/04/2012 22:00:00 UTC]] (ICME like)<br /><br />
[[04/23/2012 02:30:00 UTC]] (ICME+CIR) <br /><br />
[[06/16/2012 19:34:00 UTC]] <br /><br />
[[07/08/2012 10:00:00 UTC]] (ICME) <br /><br />
'''[[07/14/2012 17:00:00 UTC]]''' (ICME textbook event) varSITI Campaign Event<br /><br />
[[07/23/2012 23:00:00 UTC]] (STEREO-A event; extreme speed) <br><br />
[[09/30/2012 23:00:00 UTC]] (ICME, complex ejecta)<br /><br />
'''[[10/08/2012 05:00:00 UTC]]''' (ICME, "stealth" or silent) varSITI Campaign Event<br /><br />
[[10/31/2012 15:00:00 UTC]] (ICME)<br /><br />
<br />
==2013==<br />
[[02/13/2013 17:00:00 UTC]] (ICME LIKE) <br /><br />
[[02/16/2013 11:00:00 UTC]] <br /><br />
'''[[03/17/2013 05:30:00 UTC]]''' varSITI Campaign Event<br /><br />
[[04/13/2013 22:00:00 UTC]] <br /><br />
'''[[05/31/2013 15:30:00 UTC]]''' varSITI Campaign Event <br><br />
[[06/06/2013 15:00:00 UTC]] <br /><br />
[[06/27/2013 13:30:00 UTC]] <br><br />
[[07/05/2013 18:00:00 UTC]] <br><br />
[[07/09/2013 20:00:00 UTC]] <br><br />
[[07/12/2013 16:30:00 UTC]] <br><br />
[[10/01/2013 01:15:00 UTC]] <br><br />
[[12/25/2013 05:00:00 UTC]] <br><br />
<br />
==2014==<br />
[[01/08/2014-01/09/2014]] (Non-earth affecting Halo CME) <br><br />
[[02/15/2014 12:00:00 UTC]] <br><br />
[[02/19/2014 03:00:00 UTC]] <br><br />
[[02/27/2014 16:00:00 UTC]] <br><br />
[[03/25/2014 19:30:00 UTC]] <br><br />
[[04/05/2014 10:00:00 UTC]] <br><br />
[[04/07/2014 07:00:00 UTC]] <br><br />
[[04/20/2014 11:00:00 UTC]] <br><br />
[[04/29/2014 16:00:00 UTC]] <br><br />
[[05/03/2014 16:00:00 UTC]] <br><br />
[[05/07/2014 21:00:00 UTC]] <br><br />
[[05/30/2014 12:00:00 UTC]] <br><br />
[[06/07/2014 16:00:00 UTC]] <br><br />
[[09/12/2014 15:26:00 UTC]] <br></div>
Abemporad